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Molecular Gas at High Redshift
Fabian Walter, Chris Carilli, Emanuele Daddi
In order to understand galaxy evolution through cosmic times it is critical to derive the properties of the molecular gas content of galaxies, i.e. the material out of which stars…
Deep U band and R imaging of GOODS-South: Observations,data reduction and first results
M. Nonino, M. Dickinson, P. Rosati +9
We present deep imaging in the {\em U} band covering an area of 630 arcmin centered on the southern field of the Great Observatories Origins Deep Survey (GOODS). The data wer…
Journeying the Redshift Desert
Alvio Renzini, Emanuele Daddi
The cosmic star formation rate, AGN activity, galaxy growth, mass assembly and morphological differentiation all culminate at redshift . Yet, the redshift interval $1.4\lsi…
IRS Spectroscopy and Multi-wavelength Study of Luminous Star-forming Galaxies at z~1.9
J. -S. Huang, S. M. Faber, E. Daddi +24
We analyze a sample of galaxies chosen to have F24>0.5 mJy and satisfy a certain IRAC color criterion. IRS spectra yield redshifts, spectral types, and PAH luminosities, to which w…
The SINS Survey: Broad Emission Lines in High-Redshift Star-Forming Galaxies
Kristen L. Shapiro, Reinhard Genzel, Eliot Quataert +19
High signal-to-noise, representative spectra of star-forming galaxies at z~2, obtained via stacking, reveal a high-velocity component underneath the narrow H-alpha and [NII] emissi…